Annotation
In this paper the two-dimensional problem is solved for the magnetosphere of a relativistic compact star. The direct and reverse currents in the magnetotail are calculated, as well as the force exerted by the magnetic field on the edge of the current layer. The dependence of the solution on the parameters of the model is investigated.
Received: 2010 May 11
Approved: 2011 April 13
PACS:
97.10.Ex Stellar atmospheres
97.10.Ld Magnetic and electric fields; polarization of starlight
97.10.Ld Magnetic and electric fields; polarization of starlight
© 2016 Publisher M.V.Lomonosov Moscow State University
Authors
I.V. Oreshina, B.V. Somov
State Astronomical Institute, Moscow, Russia
State Astronomical Institute, Moscow, Russia
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